Muscle-to-Bone Ratio in NCAA Division I Collegiate Football Players by Position

Dengel, DR, Studee, HR, Juckett, WT, Bosch, TA, Carbuhn, AF, Stanforth, PR, and Evanoff, NG. Muscle-to-bone ratio in NCAA Division I collegiate football players by position. J Strength Cond Res 38(9): 1607-1612, 2024-The purpose of this study was to compare the muscle-to-bone ratio (MBR) in National Collegiate Athletic Association Division I football players (collegiate football players [CFP]) to healthy, age-matched controls. In addition, we examined MBR in CFP by position. A total of 553 CFP and 261 controls had their total and regional lean mass (LM), fat mass (FM), and bone mineral content (BMC) determined by dual x-ray absorptiometry (DXA). College football players were categorized by positions defined as offensive linemen (OL), defensive linemen (DL), tight end, linebacker (LB), running back (RB), punter or kicker, quarterback (QB), defensive back (DB), and wide receiver (WR). There were significant differences between CFP and controls for total LM (80.1 +/- 10.0 vs. 56.9 +/- 7.8 kg), FM (22.2 +/- 12.5 vs. 15.2 +/- 7.1 kg), and BMC (4.3 +/- 0.5 vs. 3.1 +/- 0.5 kg). Although there were significant differences in body composition between CFP and controls, there was no significant differences in total MBR between CFP and controls (18.6 +/- 1.4 vs. 18.8 +/- 1.7). Regionally, CFP had significantly lower trunk MBR than controls (26.7 +/- 2.7 vs. 28.7 +/- 4.2), but no difference was seen in leg or arm MBR. Positional differences in CFP were noted as total MBR being significantly higher in DL (19.0 +/- 1.4) than in DB (18.1 +/- 1.3), WR (18.1 +/- 1.3), and LB (18.2 +/- 1.3). OL had a significantly higher total MBR (19.2 +/- 1.3) than DB (18.1 +/- 1.3), LB (18.2 +/- 1.3), QB (18.1 +/- 1.0), and WR (18.1 +/- 1.3). In addition, RB had significantly higher total MBR (18.8 +/- 1.3) than DB (18.1 +/- 1.3) and WR (18.1 +/- 1.3). This study may provide athletes and training staff with normative values when evaluating total and regional MBR with DXA.